Table 2: Members of the identified moving group.
Name [Fe/H] $\alpha$ (J2000) $\delta$ (J2000) D U V+220 W

(dex) (h m s) (d m s) (kpc) (km s^-1) (km s^-1) (km s^-1)

BPS CS 30339-0037 -2.13 00 20 28.90 -36 12 00.7 $0.80\pm 0.16$ $-292\pm 54$ 7 $3\pm 36$ $214\pm 12$

HD 214161 -2.16 22 37 08.04 -40 30 38.4 $0.62\pm 0.12$ $-290\pm 23$ $123\pm 22$ $262\pm 15$

V^* RZ Cep -1.77 22 39 13.05 +64 51 28.9 $0.41\pm 0.08$ $-301\pm 62$ $101\pm 27$ $240\pm 47$

**Table 2:** Members of the identified moving group.
Name	[Fe/H]	$\alpha$ (J2000)	$\delta$ (J2000)	D	U	V+220	W
	(dex)	(h m s)	(d m s)	(kpc)	(km s^-1)	(km s^-1)	(km s^-1)
BPS CS 30339-0037	-2.13	00 20 28.90	-36 12 00.7	$0.80\pm 0.16$	$-292\pm 54$	7 $3\pm 36$	$214\pm 12$
HD 214161	-2.16	22 37 08.04	-40 30 38.4	$0.62\pm 0.12$	$-290\pm 23$	$123\pm 22$	$262\pm 15$
V^* RZ Cep	-1.77	22 39 13.05	+64 51 28.9	$0.41\pm 0.08$	$-301\pm 62$	$101\pm 27$	$240\pm 47$

Source LaTeX | All tables | In the text

	1 Introduction
	2 Halo samples from the Beers et al. (2000) catalog
	3 Kinematic analysis
	4 Comparison to the theory: simulations
	5 Adiabatic invariants
	6 Conclusions
	References